ITU-R S 1523-2001 Methodology for performing parametric evaluation studies of interference sensitivity for geostationary-satellite orbit fixed-satellite service systems sharing spe.pdf

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1、 Rec. ITU-R S.1523 1 RECOMMENDATION ITU-R S.1523 Methodology for performing parametric evaluation studies of interference sensitivity for geostationary-satellite orbit fixed-satellite service systems*sharing spectrum in bands above 10 GHz (Question ITU-R 236/4) (2001) The ITU Radiocommunication Asse

2、mbly, considering a) that geostationary-satellite orbit fixed-satellite service (GSO FSS) systems may operate, and many GSO FSS earth stations are located in urban areas; b) that GSO FSS systems share spectrum with other GSO FSS, non-GSO FSS and FS systems; c) that there is a need for the adequate p

3、rotection of existing GSO FSS systems, and allow the development of new GSO technologies in both non-planned bands and bands where plans exist; d) that the short-term performance of links operating in bands above 10 GHz are primarily a function of rain fade and interference; e) that the performance

4、of GSO FSS systems operating above 10 GHz is dependent on earth station location (altitude, rain rate, and elevation angle in the direction of the satellite), the receiver system temperature, the link availability, and the excess link margin; f) that to ensure a thorough consideration of the impact

5、of GSO FSS systems it is necessary to take into account differences; g) that parametric studies may be useful for assessing the impact of interference on a variety of GSO links that are, or could be located in parts of the Earth in view of the GSO orbits; h) that in many situations the modelling of

6、interference as thermal noise into GSO links is an acceptable approximation, recommends 1 that for parametric studies of GSO FSS link budgets, interference should be modelled as additive thermal noise and that generic parameters can be used as shown in Annex 1; 2 that the development of a parametric

7、 study of GSO FSS link budgets could be based on links terminating in urban centres (see Annex 2); 3 that studies involving the assessment of time varying interference sources on GSO FSS systems should take into account the effects of rain fading by utilizing the methodologies described _ *Such a sy

8、stem would consist of several GSO satellites, which together provide service and may or may not be connected via inter-satellite links. However, the methodology described herein may also be used for calculations involving a network including only one GSO satellite. 2 Rec. ITU-R S.1523 in Recommendat

9、ion ITU-R S.1323. (This Recommendation is not intended to replace network-by-network frequency coordination); 4 that the performance objectives for GSO FSS links be calculated with and without interference to determine the percentage change in the unavailability due to the interference; 5 that in or

10、der to assess the impact of interference limits on all possible GSO FSS links the analysis should consider the effects in each separate rain region. ANNEX 1 Methodology for conducting parametric studies of the effects of time varying interference on GSO FSS networks Introduction In many ITU studies,

11、 interference can be modelled as additive thermal noise. For these studies it is valid to use the reduced set of parameters, in recommends 1, to model the GSO FSS link. This link description lends itself to parametric study because it requires few input parameters. These input parameters include: ea

12、rth station altitude, latitude, rain rate, angle to the GSO satellite, receive antenna polar-ization (circular, vertical, or horizontal), receive system temperature, receive frequency and receive antenna diameter; short-term performance objective for the link; link margins that are required to meet

13、the short-term performance objective of the link. Sensitivity analysis can be performed on each input separately and the results compiled for a representative sample distribution of GSO links. This type of analysis provides a complete description of the impact of interference on the entire potential

14、 of the GSO FSS industry. The system temperature is a total system temperature and includes all noise and interference contributions in the full link budget. For a calculation of uplink interference, into the GSO satellite, the earth station is the transmitter and the receiver is on the satellite. F

15、or a calculation of downlink interference the receiver is at the earth station. For processing satellites uplinks and downlinks can be analysed separately. For transparent satellite systems the downlink system temperature includes the uplink contribution. Specifically, the calculation of the total n

16、oise temperature of the satellite (uplink), Tsat(K), and total noise earth station temperatures, Te/s(K), can be derived from the following equations: Rec. ITU-R S.1523 3 GfaGfaGfaGfaGfaGfaGfaGfaGfaGfaGfaGfaGfbGf9GeaGeaGeaGeaGeaGeaGeaGeaGeaGeaGeaGeaGebGe9+=Gf7Gf7Gf8Gf6Ge7Ge7Ge8Ge6Gf7Gf8Gf6Ge7Ge8Ge6G

17、f7Gf7Gf8Gf6Ge7Ge7Ge8Ge6Gf7Gf8Gf6Ge7Ge8Ge6Gf7Gf7Gf8Gf6Ge7Ge7Ge8Ge6Gf7Gf8Gf6Ge7Ge8Ge6Gf7Gf7Gf8Gf6Ge7Ge7Ge8Ge6Gf7Gf7Gf8Gf6Ge7Ge7Ge8Ge6Gf7Gf7Gf8Gf6Ge7Ge7Ge8Ge6Gf7Gf7Gf8Gf6Ge7Ge7Ge8Ge6Gf7Gf7Gf8Gf6Ge7Ge7Ge8Ge6Gf7Gf8Gf6Ge7Ge8Ge6BkTFRCCFSCCASICCRxXpolCCNTxXpolCCIMCCsat1.01.01.01.01.01.01.010101010101010K (1

18、) GfaGfaGfaGfaGfaGfaGfaGfaGfaGfaGfaGfaGfaGfbGf9GeaGeaGeaGeaGeaGeaGeaGeaGeaGeaGeaGeaGeaGebGe9+=Gf7Gf7Gf8Gf6Ge7Ge7Ge8Ge6Gf7Gf7Gf8Gf6Ge7Ge7Ge8Ge6Gf7Gf7Gf8Gf6Ge7Ge7Ge8Ge6Gf7Gf8Gf6Ge7Ge8Ge6Gf7Gf7Gf8Gf6Ge7Ge7Ge8Ge6Gf7Gf8Gf6Ge7Ge8Ge6Gf7Gf7Gf8Gf6Ge7Ge7Ge8Ge6Gf7Gf8Gf6Ge7Ge8Ge6Gf7Gf7Gf8Gf6Ge7Ge7Ge8Ge6Gf7Gf7Gf

19、8Gf6Ge7Ge7Ge8Ge6Gf7Gf7Gf8Gf6Ge7Ge7Ge8Ge6Gf7Gf7Gf8Gf6Ge7Ge7Ge8Ge6Gf7Gf7Gf8Gf6Ge7Ge7Ge8Ge6Gf7Gf8Gf6Ge7Ge8Ge6BkTAdjTrCCFRCCFSCCASICCRxXpolCCNTxXpolCCIMCCse1.01.01.01.01.01.01.01.0/1010101010101010K (2) where: C:the power received at the satellite (dBW) (C/IM):transmit carrier-to-intermodulation product

20、 ratio (dB) on the uplink (C/TxXpol): transmit carrier-to-transmit cross-polarization isolation ratio (dB) on the uplink N:uplink thermal noise (dBW) (C/RxXpol): carrier-to-receiver cross-polarization isolation ratio (dB) on the uplink (C/ASI): carrier-to-adjacent satellite interference ratio (dB) o

21、n the uplink (C/FS): carrier-to-fixed service interference ratio (dB) on the uplink (C/FR): carrier-to-frequency reuse isolation ratio (dB) on the uplink C: the power received at the earth station (dBW) (C/IM):transmit carrier-to-intermodulation product ratio (dB) on the downlink (C/TxXpol): transmi

22、t carrier-to-transmit cross-polarization isolation ratio (dB) on the downlink N:downlink thermal noise (dBW) 4 Rec. ITU-R S.1523 (C/RxXpol): carrier-to-receiver cross-polarization isolation ratio (dB) on the downlink (C/ASI): carrier-to-adjacent satellite interference ratio (dB) on the downlink (C/F

23、S): carrier-to-fixed service interference ratio (dB) on the downlink (C/FR): carrier-to-frequency reuse isolation ratio (dB) on the downlink (C/AdjTr): carrier-to-adjacent transponder isolation ratio (dB) on the downlink k : Boltzmans constant (W/(Hz K) B : carrier bandwidth (Hz). In the above equat

24、ions the adjacent satellite and fixed service interference are assumed to be unfaded by rain. This is a worst-case assumption that over estimates the received system temperature. For transparent satellites the total system link noise temperature, Tsys, (K) at the receive earth station including the

25、contribution of the uplink is given by: satsesysTTT +=/(3) where is the transmission gain and is equal to the numerical ratio C/C. Above 10 GHz the interference analysis should take into account the simultaneous effects due to fading and interference. Recommendation ITU-R S.1323 includes a variety o

26、f methods for combining rain fade and interference. The interference analysis results can be carried out in a variety of ways including: calculating the change in availability due to the interference as a function of rain rate; setting interference limits or assessing regional impact based on the pe

27、rcentage of links that have unacceptable interference as a function of rain rate; varying the link margin or antenna diameter to determine GSO system costs required to mitigate interference; calculating the impact of the interference versus population in urban centres. An example of a distribution o

28、f rain rates for use in performing parametric studies is shown in Annex 2. ANNEX 2 An example of a distribution of rain rates in urban areas for use in performing parametric studies Links which are the most sensitive to non-GSO interference tend to have earth stations with the following characterist

29、ics: be located in regions with low rain fall and/or at high altitude; Rec. ITU-R S.1523 5 have low receive system noise temperatures; and can meet their performance requirement when having minimum clear-sky propagation margins. In order to identify where sensitive links might exist throughout the w

30、orld, an international database of urban population areas located by: latitude, longitude, rain rate and average altitude was created. The urban population information used to create the file was derived from data provided by the Population Division, Department of Economic and Social Affairs of the

31、United Nations. Average altitude information was taken from topographical data available from the United States of America National Oceanic and Atmospheric Administration. The resulting file provides population, location, rain rate and altitude information for over 2 700 urban population centres. Th

32、e minimum population for classification as an urban centre was limited to 75 000 people (except for some few smaller island locations). The total population of the urban areas represented in the file represents about 40% of the total world population. Figure 1 graphically summarizes population in ur

33、ban centres by rain rate, and Fig. 2 graphically illustrates the number of urban areas having each rain rate. For reference, Table 1 shows the variation in urban centre altitude versus rain rate. The figures demonstrate that there are a significant number of cities with populations greater than 75 0

34、00 distributed with low rain rates. It has to be presumed that these urban areas will have satellite communication requirements similar to those of the rest of the world. 1523-0110 20 30 40 50 60 70 80 90 100 110 120 130010100150200250300350Rain fall intensity (exceeded for 0.01% of an average year)

35、 (mm/h)Urban population (million people)FIGURE 1Urban population as a function of rain rate6 Rec. ITU-R S.1523 1523-0210 20 30 40 50 60 70 80 90 100 110 120 1300100200400300800600700500Rain fall intensity exceeded for 0.01% of an average year (mm/hr)Numberofurban centresFIGURE 2Number of urban centres as a function of rain rateTABLE 1 Means of the altitudes of the urban centres for each rain rate Rain rate (mm/h) Mean (m) 10 648 20 16 30 25 40 35 50 45 60 55 70 65 80 75 90 85 100 95 110 104 120 4 130 124